Circular cosmic string loop in Brans-Dicke theory

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/3274

Full metadata record

DC Field	Value	Language
dc.creator	Barros A.	-
dc.creator	Sen A. A.	-
dc.creator	Romero C.	-
dc.date	2001	-
dc.date.accessioned	2013-05-30T01:12:49Z	-
dc.date.available	2013-05-30T01:12:49Z	-
dc.date.issued	2013-05-30	-
dc.identifier	http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332001000300026	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2001&volume=31&issue=3&spage=507	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/3274	-
dc.description	The gravitational field of a stationary circular cosmic string loop, externally supported against collapse, is investigated in the context of Brans-Dicke theory in the weak field approximation of the field equations. The solution is quasi-conformally related to the corresponding solution in Einstein's General Relativity(GR) and goes over to the corresponding solution in GR when the Brans-Dicke parameter omega becomes infinitely large.	-
dc.publisher	Sociedade Brasileira de Física	-
dc.source	Brazilian Journal of Physics	-
dc.title	Circular cosmic string loop in Brans-Dicke theory	-
Appears in Collections:	Physics and Astronomy

Files in This Item:

There are no files associated with this item.

DSpace JSPUI